Insights from JWST observations suggest that active galactic nuclei feedback evolved from a
short-lived, high-redshift phase in which radiatively cooled turbulence and/or momentum …

We summarize what large surveys of the contemporary Universe have taught us about the
physics and phenomenology of the processes that link the formation and evolution of …

Pressure-regulated star formation is a simple variant on the usual supernova-regulated star
formation efficiency that controls the global star formation rate as a function of cold gas …

Supermassive black hole feedback is thought to be responsible for the lack of star formation,
or quiescence, in a significant fraction of galaxies. We explore how observable correlations …

Supermassive black holes grow at the centre of galaxies in consonance with them. In this
Review Article, we discuss the mass-feeding mechanisms that lead to this growth in active …

Supermassive black holes (SMBHs) that reside at the centres of galaxies can inject vast
amounts of energy into the surrounding gas and are thought to be a viable mechanism to …

The growth of supermassive black holes and their host galaxies are thought to be linked, but
the precise nature of this symbiotic relationship is still poorly understood. Both observations …

Relativistic outflows (mainly observed in the radio) are a characteristic feature of both
Galactic stellar-mass black holes and supermassive black holes (SMBHs). Simultaneous …

We introduce massive black holes (BHs) in the Feedback In Realistic Environments (FIRE)
project and perform high-resolution cosmological hydrodynamic simulations of quasar-mass …

Super-Eddington accretion is one scenario that may explain the rapid assembly of∼ 10 9
M⊙ supermassive black holes (BHs) within the first billion year of the Universe. This critical …